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Uniform Supersonic Chemical Reactors: 30 Years of Astrochemical History and Future Challenges

Journal

ANGEWANDTE CHEMIE-INTERNATIONAL EDITION
Volume 56, Issue 30, Pages 8618-8640

Publisher

WILEY-V C H VERLAG GMBH
DOI: 10.1002/anie.201611240

Keywords

CRESU; laboratory astrochemistry; low temperatures; reaction kinetics; reaction mechanisms

Funding

  1. Deutsche Forschungsgemeinschaft [FOR2285]
  2. French National Programme INSU-CNRS Physique et Chimie du Milieu Interstellaire
  3. French National Programme INSU-CNRS Planetologie
  4. Spanish Ministry of Economy and Competitiveness [CSD2009-00038, CGL2013-43227-R]
  5. European Research Council [SyG 610256]

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The interstellar medium is of great interest to us as the place where stars and planets are born and from where, probably, the molecular precursors of life came to Earth. Astronomical observations, astrochemical modeling, and laboratory astrochemistry should go hand in hand to understand the chemical pathways to the formation of stars, planets, and biological molecules. We review here laboratory experiments devoted to investigations on the reaction dynamics of species of astrochemical interest at the temperatures of the interstellar medium and which were performed by using one of the most popular techniques in the field, CRESU. We discuss new technical developments and scientific ideas for CRESU, which, if realized, will bring us one step closer to understanding of the astrochemical history and the future of our universe.

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